The galaxy appears as a relatively compact, elliptical-like structure, exhibiting a smooth morphology with a concentrated central bulge. The color profile suggests a dominant population of older stars, indicated by the yellow-red hue. There is little evidence of spiral arm structure or dust lanes. The overall shape is predominantly round with slight deviation. There are no apparent signs of major tidal disturbances or ongoing mergers, though a possible minor asymmetry or faint extension cannot be fully ruled out given the image resolution. The galaxy's luminosity suggests a moderately high mass, consistent with a massive elliptical. Given the color and apparent lack of active star formation, this galaxy is likely undergoing passive evolution.
