The galaxy presents as a roughly elliptical form, though some subtle irregularities suggest possible minor disturbances in its structure, or recent merger activity. The central bulge is dominant, appearing bright and somewhat spheroidal with a yellowish hue suggestive of an older stellar population. Extending outward, there is a more diffuse region, exhibiting a greenish color. The gradient from yellow to green suggests potentially younger star formation in these outer regions. The overall morphology leans towards a smooth appearance, with a relatively concentrated central region that gives way to a less defined halo. The galaxy exhibits a moderate redshift, indicating a substantial distance.
