The galaxy presents as a largely featureless elliptical morphology, exhibiting a smooth and diffuse light distribution. The central region displays a concentrated, brighter core, suggesting a possible accumulation of older stellar populations. There is no noticeable disk structure or spiral arm patterns, indicating a relatively quiescent evolutionary state. The galaxy appears to be primarily spheroidal in shape, leaning to a round shape rather than an elongated or irregular form. There is little evidence of ongoing star formation in the image, with a predominantly yellow/red hue indicating that the dominant stellar population is comprised of older stars. There is no visible indication of any major mergers or tidal disturbances. The light falls off gradually from the core.
