The galaxy appears as a moderately bright, relatively compact object. It exhibits a generally smooth morphology, with no prominent spiral arms or bar structures readily visible. The light distribution suggests an elliptical or lenticular galaxy type. The central region appears slightly more concentrated, indicating a possible bulge. There are hints of some minor irregularities or disturbances in the outer regions of the galaxy, possibly indicative of past interactions or mergers, with no apparent major disruption. The color profile of the galaxy is relatively uniform, with a yellowish hue, which could imply an older stellar population. There appears to be limited ongoing star formation within this galaxy.
