The galaxy presents a generally smooth morphology, lacking a prominent disk or spiral arm structure. The overall shape is fairly round, exhibiting minimal elongation or asymmetry. There appears to be a central bulge that is bright, surrounded by a fainter halo of more diffuse light. The color profile indicates a redder hue in the bulge region, potentially suggestive of an older stellar population. There is some bluer color further out in the halo. There may be some evidence of minor tidal disturbances present.
