The galaxy appears as a concentrated central bulge with a smooth, luminous profile. The overall shape is somewhat elliptical, tending towards round rather than highly elongated. The color gradient suggests a population of older stars, particularly in the central region, indicated by the yellowish hue. A fainter, slightly bluer object is located in close proximity, suggesting a possible interaction or minor disturbance. There are no clearly defined spiral arms or prominent dust lanes visible. The surrounding halo exhibits a diffuse glow, with no evident signs of a major merger, although some minor disturbances cannot be ruled out. The rate of star formation within this galaxy appears to be low.
