The galaxy presents a generally smooth morphology, with a concentrated central region that gradually diffuses outwards. The light distribution appears relatively even, lacking distinct spiral arm structures or prominent star-forming regions. There are very faint hints of an extended, disk-like structure, but it is mostly homogenous. The color profile is primarily yellowish-white, suggesting an older stellar population with a lower rate of current star formation. It has a slightly elliptical shape, closer to round than cigar-shaped. There's no strong evidence of any major mergers or significant tidal disturbances. Overall, the galaxy appears to be a relatively undisturbed system, potentially an elliptical or lenticular galaxy, at an advanced stage of its evolution.
