The galaxy presents as a primarily smooth object, exhibiting an elliptical morphology. It displays a concentrated central bulge that transitions into a more diffuse halo. The light distribution suggests a relatively homogenous stellar population, with a color gradient that indicates a likely older stellar population with relatively low ongoing star formation. The shape appears to be more in between round and cigar shaped, with a tilt that allows a view of it's form. There is no obvious major disruption or presence of a companion galaxy suggestive of a recent merger. Overall, the galaxy appears as a relatively isolated and undisturbed system, consistent with a lack of significant recent interactions.
