The galaxy presents an elliptical morphology, appearing moderately elongated in shape. The light profile suggests a smooth distribution, lacking any distinct spiral arm structures or prominent dust lanes. The central bulge is prominent, exhibiting a concentrated luminosity and a yellowish hue, indicative of an older stellar population. Fainter, bluer light is visible extending outward from the bulge, suggesting a presence of younger, hotter stars in the galactic disk, but at a relatively low rate. There is some evidence of minor disturbances of galactic structure, but no significant merger events. The overall color indices suggest a system dominated by older stars, with a moderate level of on-going star formation.
