The galaxy presents as a relatively compact, elliptical structure. The light distribution appears smooth and centrally concentrated, with a gradual falloff in intensity towards the outer regions. The overall color of the galaxy is on the redder side, with a yellowish hue. This suggests a stellar population dominated by older, redder stars, indicating a cessation or significant reduction in recent star formation activity. The galaxy's shape is moderately elliptical, and its structure doesn't reveal any obvious spiral arms or prominent features indicating active star formation regions or strong dust lanes. There is no evidence of a recent or ongoing major merger.