The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish hue, suggestive of an older stellar population. The outer regions appear more diffuse, fading into the background sky. The overall shape is elongated, with a noticeable cigar-like form. There is no readily apparent disk structure, spiral arms, or signs of active star formation regions within the observed wavelengths. Likewise, there appears to be little to no evidence of significant merger activity or tidal disturbances affecting the galaxy's overall structure.
