The galaxy presents as a relatively smooth, elliptical morphology. The light distribution is centrally concentrated, exhibiting a diffuse, yellowish hue, suggestive of an older stellar population dominating the galaxy's overall light output. The shape is elongated, with the ratio of the major to minor axis approximately 2:1. There is a faint, blueish tint near the galaxy's outer edges, which could indicate the presence of younger, hotter stars forming there but it's hard to tell. There are no distinct spiral arm features or prominent dust lanes visible. There is no strong evidence of any ongoing major merging activity or tidal disturbances in the immediate vicinity.
