The galaxy presents as a luminous, slightly elongated structure, likely a disk galaxy viewed at a moderate inclination. The central bulge appears bright and concentrated, suggesting a significant population of older stars. The disk component exhibits a mottled texture, indicating the presence of both smooth regions likely composed of older stellar populations and areas with more distinct, bluer concentrations suggestive of ongoing or recent star formation. There is some indication of a faint spiral structure but it appears disturbed, with the presence of irregularities which may suggest a possible interaction or past minor merger event. There is no evidence of a prominent tidal tail or other indicators of a recent major merger. Based on its color and morphology, the galaxy appears to be undergoing a moderate level of star formation, with signs of both evolved and younger stellar populations present. Overall, the galaxy's morphology points towards a late-type spiral galaxy with indications of a disturbed structure, and moderate star formation activity.
