The galaxy presents as an elliptical or lenticular type, exhibiting a largely smooth morphology. The central bulge is prominent and displays a concentrated luminosity, appearing yellowish in color, suggesting an older stellar population. The surrounding disk, if present, is less defined but appears to be tilted relative to the observer. The galaxy shows a subtle gradient in color from the center to the outer regions, with bluer hues more apparent at the fringes. There are no readily apparent indications of recent major mergers or strong tidal disturbances, but there might be a subtle asymmetry present in the faint outer regions, potentially hinting at past minor interaction. The galaxy exhibits an estimated physical size of approximately 8.4 kpc, based on half-light radius measurements, suggesting it is an intermediate-sized system. Star formation rates appear to be relatively low, consistent with its morphology and color profile, suggesting a galaxy dominated by older stars with little active star birth occurring at the current epoch.
