The galaxy presents as a centrally concentrated object, exhibiting a smooth, elliptical morphology. The light distribution is heavily concentrated in the core, gradually fading outwards with no apparent spiral arm structure or distinct features. The color appears to be a yellowish-red hue, indicative of an older stellar population with relatively little ongoing star formation. There is no evidence of tidal tails, dust lanes, or any significant disturbances suggesting recent merger activity. The galaxy appears to be a relatively isolated system.
