The galaxy presents a generally smooth and rounded morphology. It exhibits a concentrated central region, likely indicative of a bulge. There is a notable lack of distinct spiral arm structures or prominent features, suggesting a relatively uniform stellar distribution.

The color profile of the galaxy appears to be relatively red, with subtle gradients from the center outwards. This color suggests a population of older stars. There is no evidence of active star forming regions. The estimated size of the galaxy is approximately 4 kpc.

There is no sign of any ongoing merging events or major disturbances in the galaxy's structure. Overall, the galaxy appears to be a relatively isolated and evolved system, showing the characteristics of an elliptical galaxy.
