The galaxy presents as a relatively bright, elliptical object with a smooth, concentrated central bulge exhibiting a yellow-orange hue, suggesting a population of older stars. The overall shape appears somewhat flattened, and there's evidence of a faint, extended disk component surrounding the core. This outer disk is bluer, indicating the presence of younger, hotter stars and potentially ongoing star formation. There is asymmetry in the outer disk structure suggesting minor tidal disturbances or interactions. The galaxy is relatively isolated, though there is evidence of a small object nearby that may be influencing the primary galaxy's dynamics, but it is too far to tell from the image.
