The galaxy presents as a relatively smooth, elliptical morphology. It appears to be largely featureless, with a bright central bulge that dominates the overall luminosity. There is little evidence of spiral arm structure or prominent dust lanes. The color profile suggests an older stellar population, with a redder hue indicating a lack of significant recent star formation. The galaxy's shape is elongated, but moderately so, exhibiting a form somewhere in between round and cigar-shaped. There's no obvious indication of tidal tails, disrupted morphology, or other signs of a major merger event. However, there may be a slight asymmetry visible, implying a possible minor disturbance due to a past or ongoing interaction. Overall, the galaxy appears to be a relatively quiescent system, evolving passively.