The galaxy presents as a moderately compact object with a diffuse halo. The morphology appears to be largely spheroidal in nature, with a high degree of radial symmetry. The color profile indicates a general redder hue, suggesting an older stellar population and/or significant dust obscuration. There appears to be no significant evidence of spiral arm structure or a prominent disk component, although some finer structures cannot be entirely ruled out given the image resolution. Overall, the galaxy’s light distribution is relatively smooth and featureless, but it shows some irregularities indicative of a possible ongoing or recent interaction. There appears to be some disturbance in the light profile, indicating a low level of merger activity. 
