The galaxy presents a generally smooth morphology, appearing largely featureless without a prominent disk structure. Its shape is somewhat elliptical, displaying a slight elongation rather than being perfectly circular. A concentration of light is observed towards the center, suggesting a well-defined galactic nucleus. The color profile indicates a dominant population of older stars within the galaxy, emitting a redder hue overall, particularly in the central regions. A faint, bluer halo is seen around the central bulge, suggestive of some ongoing star formation. There is no evidence of any major ongoing merger activity or significant tidal disturbance affecting the galaxy's overall structure.
