The galaxy presents as an elliptical or lenticular type, exhibiting a generally smooth, featureless morphology. The central bulge appears prominent and is a bright white color. The galaxy is generally cigar-shaped, with a ratio of minor to major axis of approximately 0.6. There is a noticeable absence of spiral arms or distinct dust lanes. No clear evidence of a recent major merger or significant tidal disruption is apparent, although a potential minor disturbance or interaction cannot be ruled out. Star formation appears subdued, as evidenced by the lack of intense blue regions. The object’s color index suggests a relatively older stellar population.
